- Open Access
Enhanced cosmic-ray antinuclei fluxes with dark matter annihilation into soft unclustered energy patterns
Phys. Rev. D 113, 115042 – Published 15 June, 2026
DOI: https://doi.org/10.1103/nf7r-rf7s
Abstract
Standard-Model (SM) hadronic parton showers initiated by secondary cosmic-ray production or dark matter (DM) annihilations robustly predict very low antinuclei yields and a strong additional suppression for heavier antinuclei. We show that an important exception can arise if DM annihilates into a confining dark sector that produces soft unclustered energy patterns (SUEPs). The hallmark of SUEPs is the emission of very large multiplicities of soft dark mesons (), which can overcome the usual phase-space suppression of antinuclei formation in parton showers, provided that the dark mesons decay promptly into SM quarks, i.e., within a SM hadronization length. We study several benchmark realizations and find that for DM masses , dark meson masses , dominantly decaying to , and a SUEP temperature , DM annihilation into SUEPs can yield tens of antideuterons and a few antihelium-3 events at at kinetic energies of and a few antideuterons and antihelium-3 events in at energies below . A future confirmation of an antinuclei signal by the or experiments could provide hints for hidden confining dynamics and would significantly constrain the relevant SUEP parameters.
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